Astronomy and Astrophysics – Astronomy
Scientific paper
Jan 2012
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012aas...21931801p&link_type=abstract
American Astronomical Society, AAS Meeting #219, #318.01
Astronomy and Astrophysics
Astronomy
Scientific paper
Low mass X-ray binary 4U 1820-30 is an 11-min period binary with two very interesting properties: a luminosity variation by factor of 2 with a period of 170 days and a negative period derivative. It has been suggested that the 170-day period in the light curve of the low mass X-ray binary 4U 1820-30 arises from the presence of a third body with a large inclination to the binary orbit. We show that this long period motion arises if the system is librating around the stable fixed point in a deep resonance. We demonstrate that mass transfer drives the system toward this fixed point, and calculate, both analytically and via numerical integrations, that the period of libration is of order 170 days when the mutual inclination is near the critical value required to induce eccentricity oscillation by the third body. The non-zero eccentricity of the binary, combined with tidal dissipation, implies that the rate of change of the binary period would be slower than, or even of opposite sign to, that implied by standard mass transfer models. If the 170-day period results from libration, then, contrary to appearances, the orbital period of the inner binary is increasing with time; in that case we can obtain a lower limit on tidal dissipation factor Q of the white dwarf secondary for the fiducial eccentricity of the inner binary. It appears unlikely that the observed negative period derivative results from the smaller than expected (but positive) value of the period derivative combined with the previously suggested acceleration of the system in the gravitational field of the host globular cluster NGC 6624.
Murray Nathan
Prodan Snezana
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